Magnetic Fields of New CP Stars Discovered with Kepler Mission Data
arXiv:2305.04898 · doi:10.1134/S1990341323020128
Abstract
The paper presents the first results of the ongoing spectropolarimetric monitoring of magnetic fields of stars, whose chemically peculiar nature has been previously revealed with the 1-m SAO RAS telescope. We selected the sample candidates using the photometric data of the Kepler and TESS space missions. The efficiency of the method of searching for new CP stars based on photometric light curves has been confirmed. We present the magnetic field measurements and estimate the atmospheric parameters of the objects under study.
arXiv commentAccepted in Astrophysical Bulletin
References in corpus (8)
- Spectroscopy Made Easy: Evolution
- The MiMeS Survey of Magnetism in Massive Stars: Introduction and overview
- B fields in OB stars (BOB): Concluding the FORS2 observing campaign
- On the detection of chemically peculiar stars using Delta a photometry
- Magnetic OB[A] Stars with TESS: probing their Evolutionary and Rotational properties (MOBSTER) - I. First-light observations of known magnetic B and A stars
- Modelling of the ultraviolet and visual SED variability in the hot magnetic Ap star CU Vir
- The Kepler view of magnetic chemically peculiar stars
- A new weak-field magnetic DA white dwarf in the local 20 pc volume. The frequency of magnetic fields in DA stars